5XMM J230457.6+122028
5XMM-DR15 stacked source · SRCID 3002554100100007
Position:
23h04m57.69s +12d20m28.8s
(346.24038°, 12.34134°)
EP flux
5.04e-14
± 2.6e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.508)
Detections
3
| SRCID | 3002554100100007 |
|---|---|
| IAUNAME | 5XMM J230457.6+122028 |
| SC_RA | 23h04m57.69s (346.24038°) |
| SC_DEC | +12d20m28.8s (12.34134°) |
| RADEC_ERR | 0.17 arcsec |
| LII / BII | 86.2893° / -42.8286° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52079.650 (2001-06-19 15:36:24.000 UTC) |
| MJD_LAST | 58269.479 (2018-05-31 11:29:14.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.04e-14 ± 2.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.65
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.22
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.64
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 4.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.86
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.25e-13 (+5.6e-13 / −5.0e-13) erg cm−2 s−1 |
|---|---|
| NH | 2.05e+21 (+2.3e+21 / −1.8e+21) cm−2 |
| Photon index (Γ) | 1.74 (+1.82 / −1.65) |
| DoF | 1183 |
| p-value | 0.804 |
| Inter-instrument norm. | 1.03 (0.97–1.10) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 13.800 (approximate flux variability amplitude) |
|---|
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.